Chapter 20 Accumulation Process of Planetesimals to the Planets : Part VI Growth of the Planets : Origin of the Solar System
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概要
- 論文の詳細を見る
Planetesimals born as a result of gravitational instability of the dust layer in the primitive solar nebula suffer successive collisions and accumulate toward the present planets. In this chapter the studies of this accumulation process, mainly numerical simulations performed in the last decade are reviewed. Direct orbital calculation of many-body system and statistical treatment in terms of mass distribution function are the two typical methods of approach. The problems included in these approaches are also discussed.
- 理論物理学刊行会の論文
- 1989-03-10
著者
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Nakagawa Y
Department Of Earth And Planetary Sciences Faculty Of Science Kobe University
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Nakagawa Yoshitsugu
Geophysical Institute University Of Tokyo
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Nakagawa Yoshitsugu
Geophysical Institute Faculty Of Science University Of Tokyo
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OHTSUKI Keiji
Geophysical Institute, University of Tokyo
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Ohtsuki Keiji
Geophysical Institute University Of Tokyo
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Ohtsuki Keiji
Geophysical Institute Faculty Of Science University Of Tokyo
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OHTSUKI Keiji
Geophysical Institute, Faculty of Science, University of Tokyo
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NAKAGAWA Yoshitsugu
Department of Physics, Kyoto University
関連論文
- Gas Drag on a Rotating Body with Gravity
- Chapter 12 Settling of Dust Particles and Formation of Planetesimals : Part IV Physical Processes in the Solar Nebula : Origin of the Solar System
- The Formation of Molecules in Contracting Interstellar Clouds
- Chapter 14 Dissipation of the Solar Nebula : Part IV Physical Processes in the Solar Nebula : Origin of the Solar System
- Origin of the Solar System : Planetary Growth in the Gaseous Nebula
- Chapter 16 Gravitational Scattering between Planetesimals and Their Statistical Behavior : Part V Physical Processes Relevant to the Planetary Growth : Origin of the Solar System
- Chapter 11 Cooling of the Solar Nebula : Part IV Physical Processes in the Solar Nebula : Origin of the Solar System
- Size Distribution of Grains Growing by Thermal Grain-Grain Collision
- Chapter 20 Accumulation Process of Planetesimals to the Planets : Part VI Growth of the Planets : Origin of the Solar System
- Statistical Behavior of Planetesimals in the Primitive Solar System
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